References quoted in the XUNDL dataset: 18NE 2H(17F,18NE):XUNDL-14

3 references found.

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1999BA49

Phys.Rev.Lett. 83, 45 (1999)

D.W.Bardayan, J.C.Blackmon, C.R.Brune, A.E.Champagne, A.A.Chen, J.M.Cox, T.Davinson, V.Y.Hansper, M.A.Hofstee, B.A.Johnson, R.L.Kozub, Z.Ma, P.D.Parker, D.E.Pierce, M.T.Rabban, A.C.Shotter, M.S.Smith, K.B.Swartz, D.W.Visser, P.J.Woods

Observation of the Astrophysically Important 3⁺ State in ¹⁸Ne via Elastic Scattering of a Radioactive ¹⁷F Beam from ¹H

NUCLEAR REACTIONS ¹H(¹⁷F, ¹⁷F), E ≈ 10-12 MeV; measured proton yields, (proton)(fluorine)-coin. ¹⁸Ne deduced resonance energy, width. ¹⁷F(p, γ), E not given; calculated resonance contribution to proton capture rate. Astrophysical implications discussed.

doi: 10.1103/PhysRevLett.83.45

2010JI02

Chin.Phys.Lett. 27, 032102 (2010)

S.-J.Jin, Y.-B.Wang, B.-X.Wang, X.-X.Bai, X.Fang, B.Guo, E.-T.Li, Y.-J.Li, Z.-H.Li, G.Lian, J.Su, s.-Q.Yan, S.Zeng, Z.-E.Yao, W.-P.Liu

Excited States in ¹⁸Ne Studied via ¹⁷F+p

NUCLEAR REACTIONS ¹H(¹⁷F, α), (¹⁷F, γ), E=55.5 MeV; measured recoil nuclei, Eα, Iα; deduced σ(θ), excitation function, ¹⁸Ne resonance states, J, π.

doi: 10.1088/0256-307X/27/3/032102

2017KU27

Phys.Rev. C 96, 045812 (2017)

S.A.Kuvin, J.Belarge, L.T.Baby, J.Baker, I.Wiedenhover, P.Hoflich, A.Volya, J.C.Blackmon, C.M.Deibel, H.E.Gardiner, J.Lai, L.E.Linhardt, K.T.Macon, B.C.Rasco, N.Quails, K.Colbert, D.L.Gay, N.Keeley

Measurement of ¹⁷F (d, n) ¹⁸Ne and the impact on the ¹⁷F (p, γ) ¹⁸Ne reaction rate for astrophysics

NUCLEAR REACTIONS ²H(¹⁷F, n)¹⁸Ne, E=95.5 MeV, [secondary ¹⁷F beam from ²H(¹⁶O, n) primary reaction using RESOLUT RIB facility at the accelerator Laboratory of Florida State University]; measured reaction products, time-of-flight, E(n), I(n), E(p), I(p), Eγ, γγ-, (particle)γ-, and (¹⁷F)p-coin using RESONEUT detector system. ¹⁸Ne; deduced center-of-mass resonance-energy spectrum from invariant-mass analysis, levels, proton resonances, J, π, σ, spectroscopic factors, Γ_p, configurations, asymptotic normalization coefficients (ANCs). Coupled reaction-channel (CRC) calculation. ¹⁷F(p, γ), T₉=0.04-0.9; deduced direct-capture reaction rates for astrophysical hot CNO cycles in novas. Comparison with previous experimental results.

doi: 10.1103/PhysRevC.96.045812